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Where do we go from here? ---- KDI ASC. Wai Mo Suen Washington University wms@wugrav.wustl.edu. The A strophysics S imulation C ollaboratory: Enabling Large Scale Simulations in Relativistic Astrophysics. PIs: U of Chicago Ian Foster Rutgers Manish Parashar UIUC Mike Norman
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Where do we go from here?---- KDI ASC Wai Mo Suen Washington University wms@wugrav.wustl.edu
The Astrophysics Simulation Collaboratory:Enabling Large Scale Simulations in Relativistic Astrophysics PIs: U of ChicagoIan Foster • RutgersManish Parashar • UIUC Mike Norman John Shalf Ed Seidel • Wash U Wai-Mo Suen (lead PI) • Potsdam Ed Seidel
Challenges of the Project (1)Build a Collaboratory based on Cactus that contains: General Relativitistic Astrophysics Codes AMR Advanced Viz Metacomputing capabilities (2) Build it as a useful tool for the whole community (3) The accretion collapse of a neutron star as the driving problem
Distribution of Effort U Chicago Meta- Computing NCSA Advanced Viz Zeus Newtonian astrophysics codes Rutgers AMR Wash U/Potsdam Einstein-GRHydro-EOS codes Accretion collapse
9/02 Physics Results Fine-tune Coordinate Control Hyperbolic Treatment of Einstiens Eqs. NS Collapse Studies Zeus 3D Fine-tune InteractiveAMR 3/01 12/99 Realistic EOS (mean field) Fine-tune Interactive Viz. GR Astro Code Codes 6/00 NS Grand Challenge (GR 3D) 5/02 5/02 3/02 Hyperbolic method study 5/02 1/00 Cactus Numerical Relativity Code Collaboratory: Phase I (Sept. 2000) Collaboratory: Phase II (Sept 2001) Collaboratory: Phase III (Sept 2002) Frameworks 5/00 5/01 5/02 Unified Data-Mgmt. Substrate DAGH + Viz. & Interection 3/02 DAGH AMR Framework Code Design Interface 5/00 5/00 5/01 5/01 12/01 3/02 Infrastructure Ubiquitous AMR Viz. Server Real-time Interactive AMR Viz. 3/02 AMR Viz. Modules (NCSA) Simulation Grid 3/02 12/00 Simulation ResrouceBroker Globus Toolkit Dynamic Code Assembler Data/Code Archive 12/00 Existing Technology Year 1 Year 2 Year 3 Roadmap
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